Characteristics of Collapse of Rotating Isothermal Clouds

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Primordial Solar Nebula Embedded in Corona
The Surface Wave Instability of Stratified Incompressible Cylinders with Differential Rotation : Astrophysics and Relativity
Numerical Simulation of Viscous Flow by Smoothed Particle Hydrodynamics : Astrophysics and Relativity
Wind from T Tauri Stars
The Structure and Evolution of Thin Viscous Disks-1-Non-steady Accretion and Excretion
Chapter 23 Gas Capture by Proto-Jupiter and Proto-Saturn : Part VI Growth of the Planets : Origin of the Solar System
Chapter 8 Efficiency of Angular Momentum Transfer by Shear Instability : Part II Formation Processes of Protostars : Origin of the Solar System
Chapter 7 Stability of the Primordial Solar Nebula : Part II Formation Processes of Protostars : Origin of the Solar System
Chapter 5 Collapse and Fragmentation of Isothermal Clouds : Part II Formation Processes of Protostars : Origin of the Solar System
Chapter 4 The Equilibrium and the Stability of Rotating Isothermal Clouds : Part II Formation Processes of Protostars : Origin of the Solar System
1. Numerical Simulation in Astrophysics : Smoothed Particle Methods (III. General Applications)
Analytic Solutions for Equilibrium of Rotating Isothermal Clouds : One-Parameter Family of Axisymmetric and Conformal Configurations
Fission of a Massive Elongated Gas Cloud Rotating at the Galactic Center
Adiabatic Collapse of Rotating Gas Clouds
Fully Three-Dimensional Hydrodynamical Collapse and Formation of Binary System
Wave Excitation in Isothermal Disks by External Gravity
Criteria for the Collapse and Fragmentation of Rotating Clouds
Three-Dimensional Hydrodynamical Simulations of Type 2 Supernova--Mixing and Fragmentation of Ejecta
Time Evolution of Pure Gravitational Waves
Excitation Energies in π-Electron Systems : Application of Green's Function Method with Second-Order Perturbaton Terms
Characteristics of Collapse of Rotating Isothermal Clouds

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